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A deep crust–mantle boundary in the asteroid 4 Vesta

Author

Listed:
  • Harold Clenet

    (EPSL, Institute of Condensed Matter Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Station 3, CH-1015 Lausanne, Switzerland)

  • Martin Jutzi

    (Physics Institute, Space Research and Planetary Sciences, Center for Space and Habitability, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland)

  • Jean-Alix Barrat

    (Université de Bretagne Occidentale, Institut Universitaire Européen de la Mer, CNRS UMR 6538, Place Nicolas Copernic, 29280 Plouzané, France)

  • Erik I. Asphaug

    (School of Earth and Space Exploration, Arizona State University, PO Box 876004, Tempe, Arizona 85287, USA)

  • Willy Benz

    (Physics Institute, Space Research and Planetary Sciences, Center for Space and Habitability, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland)

  • Philippe Gillet

    (EPSL, Institute of Condensed Matter Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Station 3, CH-1015 Lausanne, Switzerland)

Abstract

Data on Vesta’s surface material provided by the Dawn probe and impacts modelling reveals that Vesta’s crust–mantle boundary must be deeper than 80 kilometres below the surface.

Suggested Citation

  • Harold Clenet & Martin Jutzi & Jean-Alix Barrat & Erik I. Asphaug & Willy Benz & Philippe Gillet, 2014. "A deep crust–mantle boundary in the asteroid 4 Vesta," Nature, Nature, vol. 511(7509), pages 303-306, July.
    • Handle: RePEc:nat:nature:v:511:y:2014:i:7509:d:10.1038_nature13499
    DOI: 10.1038/nature13499
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